March 16: Caroline Lucretia Herschel

Caroline Lucretia Herschel

March 16, 1750 – January 9, 1848

Caroline Herschel was a German-born English astronomer, the sister of astronomer Sir William Herschel with whom she worked throughout both of their careers. Her most significant contribution to astronomy was the discovery of several comets and in particular the periodic comet 35P/Herschel-Rigollet, which bears her name.

William's interest in astronomy started as a hobby to pass time at night. He took to retiring to bed as soon as he arrived home, taking "a bason of milk" and an astronomy book for company. At breakfast the next day he would give an impromptu lecture on what he had learned the night before. Caroline became as interested as William, stating that she was "much hindered in my practice by my help being continually wanted in the execution of the various astronomical contrivances." William became known for his work on high performance telescopes, and Caroline found herself supporting his efforts.

William's telescopes gained the attention of many in the field. When comparing observations with the Astronomer Royal, Nevil Maskelyne, William's telescope proved far superior. In March 1781 he made his first observation of what would eventually prove to be the planet Uranus. In 1782, William accepted the office of King's Astronomer to George III and moved to Datchet and subsequently to Observatory House near Slough, Berkshire. The new job proved to be a mixed blessing; although it left him with ample free time to continue his astronomical observations, it also meant a reduction in income and being called upon by the king for entertainment at any time. During this time William perfected his telescope making, building a series of ever larger devices that ultimately ended with his famous 40-foot focal length instrument. Caroline was his constant assistant in his observations, also performing the laborious calculations with which they were connected. During one such observation run on the large telescope in 1783, Caroline became caught on an iron hook and when she was helped off "...they could not lift me without leaving nearly 2 ouches of my flesh behind."

In 1778 William married a rich widow. Although his new wife made every effort to stay on friendly terms with Caroline it seems her life was considerably upset. Through this period she continued her observations on her own, and made many of her discoveries. She later reconciled with the couple, and took great delight in her new nephew, John Herschel.

During her leisure hours she occupied herself with sweeping the heavens with a 27-inch focal length Newtonian telescope and by this means detected a number of astronomical objects during the years 1783 - 87, including most notably an independent discovery of M110 (NGC 205), the second companion of the Andromeda Galaxy. During 1786 - 97 she also discovered eight comets, her first comet being discovered on August 1, 1786. She had unquestioned priority on five of the comets and had rediscovered Comet Encke in 1795. The following year she was granted an annual salary of £50 by George III for her work as William's assistant.

In 1797 William's observations had shown that there were a great many discrepancies in the star catalogue published by John Flamsteed, which was difficult to use due to its having been published as two volumes, the catalogue proper and a volume of original observations. William realised that he needed a proper cross-index in order to properly explore these differences but was reluctant to devote time to it at the expense of his more interesting astronomical activities. He therefore recommended to Caroline that she undertake the task. The resulting Catalogue of Stars was published by the Royal Society in 1798 and contained an index of every observation of every star made by Flamsteed, a list of errata, and a list of more than 560 stars that had not been included.

Caroline returned to Hanover in 1822 following her brother's death, but did not abandon her astronomical studies, continuing to verify and confirm William's findings and producing a catalogue of nebulae to assist John in his work.

In 1828 the Royal Astronomical Society presented her with their Gold Medal for this work - no woman would be awarded it again until Vera Rubin in 1996.

In 1835, along with Mary Somerville, she was elected to honorary membership of the Royal Astronomical Society; they were the first honorary women members. In 1838 she was also elected as a member of the Royal Irish Academy. In 1846 at the age of 96, she was awarded the Gold Medal for Science by the King of Prussia.

March 15: Nicolas Louis de Lacaille

Abbé Nicolas Louis de Lacaille

March 15, 1713 – March 21, 1762

Abbé Nicolas Louis de Lacaille was a French astronomer. He is noted for his catalogue of nearly 10,000 southern stars, including 42 nebulous objects. This catalogue, called Coelum Australe Stelliferum, was published posthumously in 1763. It introduced 14 new constellations which have since become standard. He also calculated a table of eclipses for 1,800 years.

In honor of his contribution to the study of the southern hemisphere sky, a 60-cm telescope at Reunion Island will be named La-Caille telescope.

Born at Rumigny, in the Ardennes, he was left destitute by the death of his father, who held a post in the household of the duchess of Vendôme. Therefore, his theological studies at the College de Lisieux in Paris were undertaken at the expense of the duke of Bourbon.

After he had taken deacon's orders, however, he concentrated on science, and, through the patronage of Jacques Cassini, obtained employment, first in surveying the coast from Nantes to Bayonne, then, in 1739, in remeasuring the French arc of the meridian, for which he is honored with a pyramid at Juvisy-sur-Orge. The success of this difficult operation, which occupied two years, and achieved the correction of the anomalous result published by J. Cassini in 1718, was mainly due to Lacaille's industry and skill. He was rewarded by admission to the Academy and the appointment of mathematical professor in Mazarin college, where he worked in a small observatory fitted for his use.

His desire to observe the southern heavens led him to propose, in 1750, an astronomical expedition to the Cape of Good Hope. This was officially sanctioned by Roland-Michel Barrin de La Galissonière. Among its results were determinations of the lunar and of the solar parallax (Mars serving as an intermediary), the first measurement of a South African arc of the meridian, and the observation of 10,000 southern stars. 

Lalande said of him that, during a comparatively short life, he had made more observations and calculations than all the astronomers of his time put together. The quality of his work rivalled its quantity, while the disinterestedness and rectitude of his moral character earned him universal respect.

The crater La Caille on the Moon is named in his honor. Asteroid 9135 Lacaille (AKA 7609 P-L and 1994 EK6), discovered on October 17, 1960 by Cornelis Johannes van Houten, Ingrid van Houten-Groeneveld, and Tom Gehrels at Palomar Observatory, was also named after him.

March 14: Albert Einstein

Albert Einstein

March 14, 1879 – April 18,1955

Albert Einstein was a German-born theoretical physicist. He is best known for his theory of relativity and specifically mass–energy equivalence, expressed by the equation E = mc2. Einstein received the 1921 Nobel Prize in Physics "for his services to Theoretical Physics, and especially for his discovery of the law of the photoelectric effect."

Einstein's many contributions to physics include:

• Special theory of relativity, which reconciled mechanics with electromagnetism
  
• General theory of relativity, a new theory of gravitation which added the principle of equivalence to the principle of relativity
  
• Founding of relativistic cosmology with a cosmological constant
  
• The first post-Newtonian expansions for the perihelion advance of planet Mercury and frame-dragging
  
• The deflection of light by gravity and gravitational lensing
  
• An explanation for capillary action
  
• The first fluctuation dissipation theorem which explained the Brownian movement of molecules
  
• The photon theory and wave-particle duality from the thermodynamic properties of light
  
• The quantum theory of atomic motion in solids
  
• Zero point energy
  
• The semiclassical version of the Schrodinger equation
  
• Relations for atomic transition probabilities which predicted stimulated emission
  
• The quantum theory of a monatomic gas which predicted Bose-Einstein condensation
  
• The EPR paradox
  
• A program for a unified field theory by the geometrization of physics.
  

Einstein published over 300 scientific works and over 150 non-scientific works. In 1999 Time magazine named him the "Person of the Century", and according to Einstein biographer Don Howard, "to the scientifically literate and the public at large, Einstein is synonymous with genius."

In 1999, Albert Einstein was named "Person of the Century" by Time magazine, a Gallup poll recorded him as the fourth most admired person of the 20th century and according to The 100: A Ranking of the Most Influential Persons in History, Einstein is "the greatest scientist of the twentieth century and one of the supreme intellects of all time."

A partial list of his memorials:

• The International Union of Pure and Applied Physics named 2005 the "World Year of Physics" in commemoration of the 100th anniversary of the publication of the Annus Mirabilis Papers.
  
• The Albert Einstein Institute
  
• The Albert Einstein Memorial by Robert Berks
  
• A unit used in photochemistry, the einstein
  
• The chemical element 99, einsteinium
  
• The asteroid 2001 Einstein
  
• The Albert Einstein Award
  
• The Albert Einstein Peace Prize
  

In the period before World War II, Albert Einstein was so well-known in America that he would be stopped on the street by people wanting him to explain "that theory". He finally figured out a way to handle the incessant inquiries. He told his inquirers "Pardon me, sorry! Always I am mistaken for Professor Einstein."

Albert Einstein has been the subject of or inspiration for many novels, films, and plays. Einstein is a favorite model for depictions of mad scientists and absent-minded professors; his expressive face and distinctive hairstyle have been widely copied and exaggerated. Time magazine's Frederic Golden wrote that Einstein was "a cartoonist's dream come true."

Einstein's association with great intelligence has made the name Einstein synonymous with genius, often used in ironic expressions such as "Nice job, Einstein!".

March 13: Percival Lowell

Percival Lawrence Lowell
March 13, 1855 – November 12, 1916

Percival Lowell was a businessman, author, mathematician, and astronomer who fueled speculation that there were canals on Mars, founded the Lowell Observatory in Flagstaff, Arizona, and formed the beginning of the effort that led to the discovery of Pluto 14 years after his death. The choice of the name Pluto and its symbol were partly influenced by his initials PL.

Beginning in the winter of 1893-94, using his wealth and influence, Lowell dedicated himself to the study of astronomy, founding the observatory which bears his name. For the last 23 years of his life astronomy, the Lowell Observatory, and his and others' work at his observatory were the focal points of his life. He lived to be 61 years of age.

Lowell became determined to study Mars and astronomy as a full-time career after reading Camille Flammarion's La planète Mars. He was particularly interested in the canals of Mars, as drawn by Italian astronomer Giovanni Schiaparelli, who was director of the Milan Observatory. In 1894 Lowell chose Flagstaff, Arizona Territory as the home of his new observatory. At an altitude of over 2,100 meters (7,000 feet), with few cloudy nights, and far from city lights, Flagstaff was an excellent site for astronomical observations. This marked the first time an observatory had been deliberately located in a remote, elevated place for optimal seeing.

For the next fifteen years he studied Mars extensively, and made intricate drawings of the surface markings as he perceived them. Lowell published his views in three books: Mars (1895), Mars and Its Canals (1906), and Mars As the Abode of Life (1908). With these writings, Lowell more than anyone else popularized the long-held belief that these markings showed that Mars sustained intelligent life forms. While this idea excited the public, the astronomical community was skeptical. Many astronomers could not see these markings, and few believed that they were as extensive as Lowell claimed. As a result, Lowell and his observatory were largely ostracized. Although the consensus was that some actual features did exist which would account for these markings.

In 1909 the sixty-inch Mount Wilson Observatory telescope in Southern California allowed closer observation of the structures Lowell had interpreted as canals, and revealed irregular geological features, probably the result of natural erosion. The existence of canal-like features would not be definitively disproved until Mariner 4 took the first close-up pictures of Mars in 1965, and Mariner 9 orbited and mapped the planet in 1972. Today, the surface markings taken to be canals are regarded as an optical illusion.

Lowell's greatest contribution to planetary studies came during the last decade of his life, which he devoted to the search for Planet X, a hypothetical planet beyond Neptune. Lowell believed that the planets Uranus and Neptune were displaced from their predicted positions by the gravity of the unseen Planet X. Although Lowell's searches from 1905 to 1916 proved unsuccessful, the search continued after his death at Flagstaff in 1916.

In 1930, Clyde Tombaugh, a young astronomer recently hired by the Lowell Observatory, discovered the planet, named Pluto. Partly in recognition of Lowell's efforts, a stylized P-L monogram (the first two letters of the new planet's name and also Lowell's initials), was chosen as Pluto's astronomical symbol.

However, it would subsequently emerge that the Planet X theory was mistaken. Pluto's mass could not be determined until 1978, when a satellite was discovered. This confirmed what had been increasingly suspected: Pluto's gravitational influence on Uranus and Neptune is negligible, certainly not nearly enough to account for the discrepancies in their orbits. In 2006, after Clyde Tombaugh's death, Pluto was reclassified as a dwarf planet by the International Astronomical Union.

In addition, it is now known that the discrepancies between the predicted and observed positions of Uranus and Neptune were not caused by the gravity of an unknown planet. Rather, they were due to an erroneous value for the mass of Neptune. Voyager 2's 1989 encounter with Neptune yielded a more precise value of its mass, and the discrepancies disappear when using this value.

Although Lowell's theories of the Martian canals and of Planet X are now discredited, his practice of building observatories at the position where they would best function has been adopted as a principle. He also established the program and setting which made the discovery of Pluto by Clyde Tombaugh possible.

The Lunar crater Lowell and a crater on Mars have been named in his honor.

March 12: Simon Newcomb

Simon Newcomb

March 12, 1835 – July 11, 1909

Simon Newcomb was a Canadian-American astronomer and mathematician. Though he had little conventional schooling, he made important contributions to timekeeping as well as writing on economics, statistics and authoring a science fiction novel.

Newcomb studied mathematics and physics privately and supported himself with some school-teaching before becoming a human computer (a functionary in charge of calculations) at the Nautical Almanac Office in Cambridge, Massachusetts in 1857. At around the same time, he enrolled at the Lawrence Scientific School of Harvard University, graduating BS in 1858.

In the prelude to the American Civil War, many US Navy staff of Confederate sympathies left the service and, in 1861, Newcomb took advantage of one of the ensuing vacancies to become professor of mathematics and astronomer at the United States Naval Observatory, Washington DC. Newcomb set to work on the measurement of the position of the planets as an aid to navigation, becoming increasingly interested in theories of planetary motion.

By the time Newcomb visited Paris, France in 1870, he was already aware that the table of lunar positions calculated by Peter Andreas Hansen was in error. While in Paris, he realised that, in addition to the data from 1750 to 1838 that Hansen had used, there was further data stretching as far back as 1672. Newcomb was able to use the "new" data to revise Hansen's tables.

He was offered the post of director of the Harvard College Observatory in 1875 but declined, having by now settled that his interests lay in mathematics rather than observation.

In 1877 he became director of the Nautical Almanac Office where, ably assisted by George William Hill, he embarked on a program of recalculation of all the major astronomical constants. Despite fulfilling a further demanding role as professor of mathematics and astronomy at Johns Hopkins University from 1884, he conceived with A. M. W. Downing a plan to resolve much international confusion on the subject. By the time he attended a standardisation conference in Paris, France in May 1896, the international consensus was that all ephemerides should be based on Newcomb's calculations. A further conference as late as 1950 confirmed Newcomb's constants as the international standard.

In 1878, Newcomb had started planning for a new and precise measurement of the speed of light that was needed to account for exact values of many astronomical constants. He had already started developing a refinement of the method of Léon Foucault when he received a letter from the young naval officer and physicist Albert Abraham Michelson who was also planning such a measurement. Thus began a long collaboration and friendship. In 1880, Michelson assisted at Newcomb's initial measurement with instruments located at Fort Myer and the United States Naval Observatory, then situated on the Potomac River. However, Michelson had left to start his own project by the time of the second set of measurements between the observatory and the Washington Monument. Though Michelson published his first measurement in 1880, Newcomb's measurement was substantially different. In 1883, Michelson revised his measurement to a value closer to Newcomb's.

Awards and honours

• Member, and holder of several offices, of the National Academy of Sciences (1869);
  
• Gold Medal of the Royal Astronomical Society (1874);
  
• Fellow of the Royal Society (1877);
  
• Huygens Medal of the Haarlem Academy of Sciences (1878);
  
• Editor of the American Journal of Mathematics (1885 - 1900);
  
• Copley Medal of the Royal Society (1890);
  
• Chevalier of the Légion d'Honneur (1893);
  
• President of the American Mathematical Society (1897 - 1898);
  
• Bruce Medal of the Astronomical Society of the Pacific (1898); and
  
• Founding member and first president of the American Astronomical Society (1899 - 1905).
  
• Asteroid 855 Newcombia is named after him.
  
• The crater Newcomb on the Moon is named after him.
  
• The Royal Astronomical Society of Canada has a writing award named after him.

March 11: Urbain Le Verrier

Urbain Jean Joseph Le Verrier

March 11, 1811 – September 23, 1877

Urbain Le Verrier was a French mathematician who specialized in celestial mechanics and is best known for his part in the discovery of Neptune.

Le Verrier studied at the Ecole Polytechnique. Following a brief period studying chemistry under Gay-Lussac, Le Verrier switched to astronomy, particularly celestial mechanics. He accepted a job at the Paris Observatory, where he spent most of his professional life, and eventually became that institution's Director.

Le Verrier's most famous achievement is his prediction of the existence of the then unknown planet Neptune, using only mathematics and astronomical observations of the known planet Uranus. Encouraged by physicist Arago, Director of the Paris Observatory, Le Verrier was intensely engaged for months in complex calculations to explain small but systematic discrepancies between Uranus's observed orbit and the one predicted from the laws of gravity of Newton. 

At the same time, but unknown to Le Verrier, similar calculations were made by John Couch Adams in England. Le Verrier announced his final predicted position for Uranus's unseen perturbing planet publicly to the French Academy on August 31, 1846, two days before Adams's final solution, which turned out to be 12° off the mark, was privately mailed to the Royal Greenwich Observatory. Le Verrier transmitted his own prediction by September 18 letter to Johann Galle of the Berlin Observatory. The letter arrived five days later, and the planet was found with the Berlin Fraunhofer refractor that same evening, September 23, 1846 by Galle and Heinrich d'Arrest within 1° of the predicted location near the boundary between Capricorn and Aquarius.

There was, and to an extent still is, controversy over the apportionment of credit for the discovery. There is no ambiguity to the discovery claims of Le Verrier, Galle, and d'Arrest. Adams's work was begun earlier than Le Verrier's but was finished later and was unrelated to the actual discovery. Not even the briefest account of Adams's predicted orbital elements was published until more than a month after Berlin's visual confirmation. But Adams himself made full public acknowledgement of Le Verrier's priority and credit (not forgetting to mention the role of Galle) when he gave his paper to the Royal Astronomical Society in November 1846:

I mention these dates merely to show that my results were arrived at independently, and previously to the publication of those of M. Le Verrier, and not with the intention of interfering with his just claims to the honours of the discovery ; for there is no doubt that his researches were first published to the world, and led to the actual discovery of the planet by Dr. Galle, so that the facts stated above cannot detract, in the slightest degree, from the credit due to M. Le Verrier.

– Adams (1846)

Galvanized by his success with Neptune, Le Verrier proceeded to interpret variations in the orbit of Mercury as being due to an unknown planet, tentatively named Vulcan. This triggered a wave of false detections, which lasted until 1915, when Einstein explained Mercury's anomalous motion with his theory of general relativity.

The last quarter century of Le Verrier's life was engaged in establishing the orbits of all eight planets, a project which he only narrowly lived to see completed and printed.

Honors

• Gold Medal of the Royal Astronomical Society - 1868 and 1876
  
• Namesake of craters on the Moon and Mars, a ring of Neptune, and the asteroid 1997 Leverrier
  
• One of the 72 names engraved on the Eiffel Tower
  

March 10: MRO Attained Martian Orbit

MRO attained Martian orbit on March 10, 2006

NASA's Mars Reconnaissance Orbiter (MRO) is a multipurpose spacecraft designed to conduct reconnaissance and exploration of Mars from orbit.

When MRO entered orbit there were five other spacecraft in orbit of or on Mars: Mars Global Surveyor, Mars Express, Mars Odyssey, and two Mars Exploration Rovers; a then record for most spacecraft operational in Mars vicinity. The $720 million USD spacecraft was built by Lockheed Martin under the supervision of the Jet Propulsion Laboratory. It was launched August 12, 2005, and attained Martian orbit on March 10, 2006. In November 2006, after five months of aerobraking, it entered its final science orbit and began its primary science phase.

MRO is modeled after NASA's highly successful Mars Global Surveyor to conduct surveillance of Mars from orbit. Early specifications of the satellite included a large camera to take high resolution pictures of Mars. In this regard, Jim Garvin, the Mars exploration program scientist for NASA, proclaimed that MRO would be a "microscope in orbit". The satellite was also to include a visible-near-infrared spectrograph.

MRO contains a host of scientific instruments such as cameras, spectrometers, and radar, which are used to analyze the landforms, stratigraphy, minerals, and ice of Mars. It paves the way for future spacecraft by monitoring daily weather and surface conditions, studying potential landing sites, and hosting a new telecommunications system. MRO's telecommunications system will transfer more data back to Earth than all previous interplanetary missions combined, and MRO will serve as a highly capable relay satellite for future missions.

MRO is using its on-board scientific equipment to study the Martian climate, weather, atmosphere, and geology, and to search for signs of water in the polar caps and underground. In addition, MRO is looking for the remains of the previously lost Mars Polar Lander and Beagle 2 spacecraft, and serves as the first step in setting up an internet protocol network for the planets in our solar system. After its main science operations are completed, the probe's extended mission is to be the communication and navigation system for landers and rover probes.

March 9: David Fabricius

David Fabricius

March 9, 1564 - May 7, 1617

David Fabricius was a German theologian who made two major discoveries in the early days of telescopic astronomy, jointly with his eldest son, Johannes Fabricius (1587-1615).

David Fabricius (Latinization of his proper name David Faber or David Goldschmidt) served as pastor for small towns near his birthplace in Esens, Frisia (now northwest Germany and northeast Netherlands), at Resterhafe near Dornum in 1584 and at Osteel in 1603. As was common for churchmen of the day, he dabbled in science: his particular interest was astronomy.

Fabricius discovered the first known periodic variable star (as opposed to cataclysmic variables, such as novas and supernovas), Mira, in August of 1596. At first he believed it to be "just" another nova, as the whole concept of a recurring variable did not exist at the time. When he saw Mira brighten again in 1609, however, it became clear that a new kind of object had been discovered in the sky.

Two years later, his son Johannes Fabricius returned from university in the Netherlands with telescopes that they turned on the Sun. Despite the difficulties of observing the sun directly, they noted the existence of sunspots, the first confirmed instance of their observation (though unclear statements in East Asian annals suggest that Chinese astronomers may have discovered them with the naked eye previously, and Fabricius may have noticed them himself without a telescope a few years before). 

The pair soon invented camera obscura telescopy so as to save their eyes and get a better view of the solar disk, and observed that the spots moved. They would appear on the eastern edge of the disk, steadily move to the western edge, disappear, then reappear at the east again after the passage of the same amount of time that it had taken for it to cross the disk in the first place.

This suggested that the Sun rotated on its axis, which had been postulated before but never backed up with evidence. Johannes published Maculis in Sole Observatis, et Apparente earum cum Sole Conversione Narratio ("Narration on Spots Observed on the Sun and their Apparent Rotation with the Sun") in June of 1611. Unfortunately, the book remained obscure and was eclipsed (so to speak) by the independent discoveries of and publications about sunspots by Christoph Scheiner in January 1612 and Galileo Galilei in March 1612.

Besides these two discoveries, little else is known about David Fabricius except his unusual manner of death: after denouncing a local goose thief from the pulpit, the accused man struck him in the head with a shovel and killed him.

Copies of a map he made of Frisia in 1589 are also still extant. He is also name-checked in Jules Verne's From the Earth to the Moon as someone who claimed to have seen lunar inhabitants through his telescope, though that particular fact is merely part of Verne's fiction. In 1895 a monument was erected to his memory in the churchyard at Osteel where he was pastor from 1603 until 1617. The Lunar crater Fabricius is named in his honor. 

March 8: Alvan Clark

Alvan Clark

March 8, 1804 – August 19, 1887

Alvan Clark, born in Ashfield, Massachusetts, the descendant of a Cape Cod whaling family of English ancestry, was an American astronomer and telescope maker. 

He was a portrait painter and engraver, but at the age of 40 become involved in telescope making. Using glass blanks made by Chance Brothers of Birmingham and Feil-Mantois of Paris, his firm Alvan Clark & Sons ground lenses for refracting telescopes, including the largest in the world at the time: 

• the 18.5-inch (470 mm) at Dearborn Observatory at the Old University of Chicago (the lens was originally intended for Ole Miss) 
  
• the 26-inch (660 mm) at the United States Naval Observatory, 
• the 30-inch (760 mm) at Pulkovo Observatory (destroyed in the Siege of Leningrad; only the lens survives) 
  
• the 36-inch (910 mm) telescope at Lick Observatory (still third-largest) 
  
• the 40-inch (1,000 mm) at Yerkes Observatory, which remains the largest successful refracting telescope in the world
  

He was the first person in the United States to make achromatic lenses, and the most important modern telescopes have been constructed at his factory in Cambridge-port. Mr. Clark invented numerous improvements in telescopes and their manufacture, including the double eye-piece, an ingenious method of measuring small celestial arcs. A list of discoveries made by him with telescopes of his own manufacture is given in the "Proceedings of the Royal Astronomical Society" (London, vol. 17, No. 9).

Mr. Clark accompanied the total-eclipse expedition to Jerez, Spain, in 1870, and also the similar expedition to Wyoming in 1878. As an independent observer he has discovered fourteen intricate double stars, including the companion to Sirius, for which the Lalande gold medal was awarded him by the French academy of sciences in 1862. He has also made numerous inventions connected with the manufacture of refracting telescopes. 

One of Clark's sons, Alvan Graham Clark, discovered the dim companion of Sirius. His other son was George Bassett Clark; both sons were partners in the firm.

The Lunar crater Clark and on Mars are named in his honor.

March 7: John Herschel

Sir John Frederick William Herschel

March 7, 1792 – May 11, 1871

Sir John Frederick William Herschel, 1st Baronet KH, FRS, was an English mathematician, astronomer, chemist, and experimental photographer/inventor, who in some years also did valuable botanical work. He was the son of astronomer Sir William Herschel and the father of 12 children.

Herschel originated the use of the Julian day system in astronomy. He named seven moons of Saturn and four moons of Uranus. He made many contributions to the science of photography, and investigated colour blindness and the chemical power of ultraviolet rays.

Herschel studied at Eton College and St John's College, Cambridge. It was during his time as an undergraduate that he became friends with Charles Babbage and George Peacock. He took up astronomy in 1816, building a reflecting telescope with a mirror 18 inches (460 mm) in diameter and with a 20-foot (6.1 m) focal length. Between 1821 and 1823 he re-examined, with James South, the double stars catalogued by his father. For this work he was presented in 1826 with the Gold Medal of the Royal Astronomical Society (which he won again in 1836), and with the Lalande Medal of the French Institute in 1825, while in 1821 the Royal Society bestowed upon him the Copley Medal for his mathematical contributions to their Transactions. Herschel was made a Knight of the Royal Guelphic Order in 1831.

Declining an offer from the Duke of Sussex that they travel to South Africa on a Navy ship, Herschel and his wife paid ₤500 for passage on the 'S.S. Mountstuart Elphinstone', a ship of 611 tons, which departed from Portsmouth on 13 November 1833. The voyage to South Africa was made in order to catalogue the stars, nebulae, and other objects of the southern skies. This was to be a completion as well as extension of the survey of the northern heavens undertaken initially by his father William Herschel. He arrived in Cape Town on 15 January 1834 and set up a private 21 ft (6.4 m) telescope at Feldhausen at Wynberg. Amongst his other observations during this time was that of the return of Comet Halley. Herschel collaborated with Thomas Maclear, the Astronomer Royal at the Cape of Good Hope, and the two families became close friends.

Herschel wrote many papers and articles, including entries on meteorology, physical geography and the telescope for the eighth edition of the Encyclopædia Britannica. He also translated The Iliad of Homer.

He proposed a correction to the Gregorian calendar, making years that are multiples of 4,000 not leap years, thus reducing the average length of the calendar year from 365.2425 days to 365.24225. Although this is closer to the mean tropical year of 365.24219 days, his proposal has never been adopted because the Gregorian calendar is based on the mean time between vernal equinoxes (currently 365.2424 days).

In 1835, the New York Sun newspaper wrote a series of satiric articles that came to be known as the Great Moon Hoax, with statements falsely attributed to Herschel about his supposed discoveries of animals living on the Moon, including batlike winged humanoids.

Herschel Island (in the Arctic Ocean, north of the Yukon Territory), Mount Herschel (in Antarctica) and the crater J. Herschel on the Moon are named in his honor.

March 6: Joseph von Fraunhofer

Joseph von Fraunhofer

March 6, 1787 – June 7, 1826

Joseph von Fraunhofer was a German optician. He is known for the discovery of the dark absorption lines known as Fraunhofer lines in the Sun's spectrum, and for making excellent optical glass and achromatic telescope objectives.

Fraunhofer was born in Straubing, Bavaria. He became an orphan at the age of 11, and he started working as an apprentice to a harsh glassmaker named Philipp Anton Weichelsberger. In 1801 the workshop in which he was working collapsed and he was buried in the rubble. The rescue operation was led by Maximilian IV Joseph, Prince Elector of Bavaria (the future Maximilian I Joseph). The prince entered Fraunhofer's life, providing him with books and forcing his employer to allow the young Joseph Fraunhofer time to study.

After eight months of study, Fraunhofer went to work at the Optical Institute at Benediktbeuern, a secularised Benedictine monastery devoted to glass making. There he discovered how to make the world's finest optical glass and invented incredibly precise methods for measuring dispersion. In 1818 he became the director of the Optical Institute. Due to the fine optical instruments he had developed, Bavaria overtook England as the centre of the optics industry. Even the likes of Michael Faraday were unable to produce glass that could rival Fraunhofer's.

His illustrious career eventually earned him an honorary doctorate from the University of Erlangen in 1822. In 1824, he was awarded the order of merit, became a noble, and made an honorary citizen of Munich. Like many glassmakers of his era who were poisoned by heavy metal vapours, Fraunhofer died young, in 1826 at the age of 39. His most valuable glassmaking recipes are thought to have gone to the grave with him.

In 1814, Fraunhofer invented the spectroscope, and discovered 574 dark lines appearing in the solar spectrum. These were later shown to be atomic absorption lines, as explained by Kirchhoff and Bunsen in 1859. These lines are still called Fraunhofer lines in his honour.

He also invented the diffraction grating and in doing so transformed spectroscopy from a qualitative art to a quantitative science by demonstrating how one could measure the wavelength of light accurately. He found out that the spectra of Sirius and other first-magnitude stars differed from each other and from the sun, thus founding stellar spectroscopy.

Ultimately, however, his primary passion was still practical optics, once noting that

"In all my experiments I could, owing to lack of time, pay attention to only those matter which appeared to have a bearing upon practical optics."

In the early 1990s a firm that designed and built refracting telescopes was named in his honor Fraunhofer Systems Company since the telescopes were based on his design but now the company is part of Burbank Optical Company.

The Lunar crater Fraunhofer is named in his honor.

March 5: James Bradley

James Bradley

March 1693 – July 13, 1762

(exact date of birth is unknown)

James Bradley was an English astronomer and Astronomer Royal from 1742. He is best known for discovering the aberration of light while attempting to detect stellar parallax.

Bradley entered Balliol College, Oxford, on March 15, 1711, and took degrees of B.A. and M.A. in 1714 and 1717 respectively. His early observations were made at the rectory of Wanstead in Essex, under the tutelage of his uncle, the Rev. James Pound, himself a skilled astronomer, and was elected a fellow of the Royal Society on November 6, 1718. In 1721 he was appointed to the Savilian chair of astronomy at Oxford.

Bradley worked with Samuel Molyneux until Molyneux's death in 1728 trying to measure the parallax of Gamma Draconis. However, while not finding the expected parallax, they instead found an unexplained motion which shortly after Molyneux's death Bradley realized was caused by the aberration of light. The discovery of the aberration of light, which was conclusive evidence for the movement of earth and hence the correctness of Aristarchus and Kepler's theories, was announced to the Royal Society in January 1729. 

The measurement of parallax had been the Holy Grail of astronomers since the time of Aristarchus and Archimedes. If the Earth orbited round the Sun, as postulated by Aristarchus and formulated much later by Copernicus, then nearby stars should show some apparent change of position over an annual cycle because of the changed viewpoint from the Earth at each extreme of its orbit. This is the same effect as when nearby objects seen from the window of a moving train, appear to change position much faster than distant objects — ‘parallax’.

Unfortunately for Helio-centrists (notably Galileo), the best endeavours of astronomers for centuries had produced no reliable evidence whatsoever of stellar parallax — just as expected by the Geo-centrists: if the Earth was stationary at the centre of the universe then of course the stars would not show any change of position.

The best the Helio-centrists could do was to argue that the stars were so hugely distant that the parallax effect was tiny and beyond the ability of present instruments to detect. Succeeding generations worked to build better instruments and devise new strategies for measurement. When Bradley had directly detected the effect of the Earth’s motion around the Sun, Aristarchus, Copernicus and Galileo were vindicated:

“eppur si muove” — and yet it does move.

This aberration also allowed Bradley to accurately estimate the speed of light which had previously been shown to be finite by the work Ole Rømer and others. The observations upon which it was founded were made at Molyneux’s house on Kew Green. Bradley did not announce the supplementary detection of nutation until February 14, 1748, when he had tested its reality by minute observations during an entire revolution (18.6 years) of the moon’s nodes. 

In 1742, he had been appointed to succeed Edmund Halley as Astronomer Royal; his enhanced reputation enabled him to apply successfully for a set of instruments costing GB£1,000; and with an 8-foot quadrant completed for him in 1750 by John Bird, he accumulated at Greenwich in ten years materials of inestimable value for the reform of astronomy. A crown pension of GB£250 a year was conferred upon him in 1752.

He died on July 13, 1762. The publication of his observations was delayed by disputes about their ownership; but they were finally issued by the Clarendon Press, Oxford, in two folio volumes (1798, 1805). The insight and industry of Friedrich Wilhelm Bessel were, however, needed for the development of their fundamental importance.

The Lunar promontory Mons Bradley is named in his honor.

March 4: Sir Alfred Patrick Caldwell-Moore

Sir Alfred Patrick Caldwell-Moore

b. March 4, 1923

Patrick Moore, CBE, HonFRS, FRAS, is an English amateur astronomer who has attained prominent status in astronomy as a writer, researcher, radio commentator and television presenter of the subject and who is credited as having done more than any other to raise the profile of astronomy among the British general public. 

Sir Patrick is a former president of the British Astronomical Association, co-founder and former president of the Society for Popular Astronomy, author of over 70 books on astronomy, presenter of the longest running television series (with the same original presenter), The Sky at Night on the BBC and a famous figure on British television. He is well known for his rapid mode of speech, trademark monocle, poorly fitting blazers, extremely high trouser line and a fondness for the xylophone.

Sir Patrick is also an accomplished composer. He is entirely self-taught in music. His favourite genres include 19th century Viennese waltzes and marches, but he has also turned to ragtime, polkas, and a nocturne. In 1981 he played a xylophone solo in a Royal Command Performance.

He developed an interest in astronomy at the age of six and was elected to the British Astronomical Association at the age of 11. Moore eventually set up home at Selsey in Sussex, where he constructed a home-made reflecting telescope in his garden and began to observe the Moon. He was fascinated by the subject and he is now acknowledged as a specialist in lunar observation, one of his particular areas of expertise being the study of the glimpses of the Moon's far side that are occasionally visible due to the Moon's libration. He was also an early observer of Transient lunar phenomena: short-lived glowing areas on the lunar surface.

On 26 April 1957, at 10:30 pm, in an event that was to be a landmark of his career, Moore presented the first episode of The Sky at Night, a BBC television programme for astronomy enthusiasts. Since then, he has presented every episode each month, excepting July 2004, because of a near-fatal bout of food poisoning.

Patrick Moore has undertaken significant research in astronomy. In 1959, the Soviet Union used his charts of the moon to correlate their first pictures of the far side with his mapped features on the near side and he was involved in the lunar mapping used by the NASA Apollo space missions. In 1965, he was appointed Director of the newly-constructed Armagh Planetarium, a post he held until 1968. During the Apollo program, Moore was a presenter of the BBC's television's coverage of the moon landing missions. He compiled the Caldwell catalogue of astronomical objects and in 1982 asteroid 2602 Moore was named in his honour.

Moore has written over 70 books on astronomy, all of them typed on a Woodstock typewriter of 1908 vintage, which he has always preferred to any more modern device. After the BBC withdrew financial support, he independently produced a 50th anniversary DVD of his life and work titled 'The Astronomical Patrick Moore'.

In 1945, Moore was elected a Fellow of the Royal Astronomical Society. In 1968, he was appointed OBE and advanced to CBE in 1988. In 2001, he was knighted as a Knight Bachelor "for services to the popularisation of science and to broadcasting". In the same year, he was appointed an Honorary Fellow of the Royal Society. In June 2002, he was appointed as Hon. Vice President of the Society for the History of Astronomy.

During a podcast of The Ricky Gervais Show in 2006, he was chosen by Karl Pilkington as one of six people who ought to re-start and educate human life on an imaginary uninhabited planet.

March 3: Ralph Asher Alpher

Ralph Asher Alpher

March 3, 1921 - August 12, 2007

Ralph Alpher was an American physicist best known for his theoretical work on the origin and early evolution of the Universe. In 1948, together with Hans Bethe and George Gamow, he suggested how the abundances of chemical elements could be explained as a result of thermonuclear processes immediately after the Big Bang. This work became known as the “alpha, beta, gamma” theory. As further developed in collaborations with Robert Herman and others, this concept of cosmic nucleosynthesis became an integral part of the standard Big Bang model. It also led to a prediction of the cosmic microwave background. 

Alpher earned his bachelor's degree and advanced graduate degrees in physics from George Washington University, all the while working as a physicist on contract to the Navy, and eventually for the Johns Hopkins University Applied Physics Laboratory. He met eminent Russian physicist George Gamow at the University, who subsequently took him on as his doctoral student. This was somewhat of a coup, as Gamow was an eminent Soviet defector and one of the luminaries on the GWU faculty. It is apparent that Alpher provided much needed mathematical ability to support Gamow's theorizing.

Alpher's dissertation in 1948 dealt with a subject that came to be known as Big Bang nucleosynthesis. The Big Bang is a term coined initially in derision by Fred Hoyle to describe the cosmological model of the universe as expanding into its current state from a primordial condition of enormous density and temperature. Nucleosynthesis is the explanation of how more complex elements are created out of simple elements in the moments following the Big Bang. Right after the Big Bang, when the temperature was extremely high, if any nuclear particles such as neutrons and protons, became bound together (being held together by the attractive nuclear force) they would be immediately broken apart by the high energy photons(quanta of light) present in high density. In other words, at this extremely high temperature, the photons' kinetic energy would overwhelm the binding energy of the strong nuclear force. For example, if a proton and a neutron became bound together (forming deuterium), it would be immediately broken apart by a high energy photon. However, as time progressed, the universe expanded and cooled and the average energy of the photons decreased. At some point, roughly one second after the Big Bang, the attractive force of nuclear attraction would begin to win out over the lower energy photons and neutrons and protons would begin to form stable deuterium nuclei. As the universe continued to expand and cool, additional nuclear particles would bind with these light nuclei, building up heavier elements such as helium, etc. Alpher argued that the Big Bang would create hydrogen, helium and heavier elements in the correct proportions to explain their abundance in the early universe. Alpher and Gamow's theory originally proposed that all atomic nuclei are produced by the successive capture of neutrons, one mass unit at a time. However, later study challenged the universality of the successive capture theory since no element was found to have a stable isotope with an atomic mass of five or eight, hindering the production of elements beyond helium.

Since this dissertation was (correctly) perceived to be ground-breaking, over 300 people attended the dissertation defense, including the Press, and articles about his predictions and a Herblock cartoon appeared in major newspapers. This was quite unusual for a doctoral dissertation. Later the same year, collaborating with Dr. Robert Herman, Alpher predicted the temperature of the residual radiation (known as cosmic background radiation) resulting from the hypothesized Big Bang. However, Alpher's predictions concerning the comsic background radiation were more or less forgotten and they were rediscovered by Robert Dicke and Yakov Zel'dovich in the early 1960s. The existence of the cosmic background radiation and its temperature were measured experimentally in 1964 by two physicists working for Bell Laboratories in New Jersey, Arno Penzias and Robert Wilson, who were awarded the Nobel prize in physics for this work in 1978. 

Although his name appears on the paper, Hans Bethe had virtually no part in the development of the theory, although he later worked on related topics; Gamow added his name to make the seminal paper's title a pun on "Alpha-Beta-Gamma" (α,β,γ), the first three letters of the Greek alphabet. Thus, Alpher's independent dissertation was first published on April 1, 1948 in the Physical Review with three authors.

Alpher and Robert Herman were later awarded the Henry Draper Medal in 1993. They were also awarded the Magellanic Premium of the American Philosophical Society in 1975, the Georges Vanderlinden Physics prize of the Belgian Academy of Sciences, as well as significant awards of the New York Academy of Sciences and the Franklin Institute of Philadelphia — in other words, nearly every significant professional recognition saving the Nobel Prize. Two Nobel Prizes in physics have been awarded for empirical work related to the cosmic background radiation — in 1978 to Arno Penzias and Robert Wilson and in 2006 to John Mather and George Smoot. Alpher and Herman (the latter, posthumously) published their own account of their work in cosmology in 2001, Genesis of the Big Bang (Oxford University Press). Alpher's seminal work was finally recognized in 2005 when he was awarded the National Medal of Science (the Nation's highest scientific honor). The citation for the award reads

"For his unprecedented work in the areas of nucleosynthesis, for the prediction that universe expansion leaves behind background radiation, and for providing the model for the Big Bang theory."

The medal was presented to his son Dr. Victor S. Alpher on July 27, 2007 by President George W. Bush, as his father could not travel to receive the award. 

March 2: Vladimír Remek

Vladimír Remek

b. September 26, 1948

March 2, 1978 - the first man in space who was 

neither a US nor Soviet citizen.

Vladimír Remek is the first Czechoslovak in space (son of Czech mother and Slovak father), and the first cosmonaut from a country other than the Soviet Union or the United States. As of 2004, with the entry of the Czech Republic into the European Union Vladimír Remek is considered to be the first European Astronaut. He flew aboard Soyuz 28 from March 2nd to March 10th 1978, for seven days, 22 hours, and 17 minutes. In later life he became a politician and now sits in the European Parliament.

Remek was born in České Budějovice. He graduated from the Air Force Academy and worked as an Air Force pilot. He joined the Intercosmos program as an Army pilot in 1976.

Vladimír Remek was awarded the title Hero of the Soviet Union on March 16, 1978. Later, he became director of the Museum for Aviation and Astronautics in Prague, then representative for the company ČZ in Moscow. He later worked at the Czech embassy in Russia.

He is now a Member of the European Parliament for the Communist Party of Bohemia and Moravia, which is part of the European United Left–Nordic Green Left party group in the European Parliament. He is married and has one child.

The asteroid 2552 Remek is named after him.

"From planets to the Parliament: Vladimír Remek - MEP, Cosmonaut"

March 1: George Ogden Abell

George Ogden Abell

March 1, 1927 – October 7, 1983

George Abell was an astronomer at UCLA. He worked as a research astronomer, teacher, administrator, popularizer of science and education, and skeptic. Abell received his B.S. (1951), M.S. (1952) and Ph.D. (1957) from the California Institute of Technology. He began his astronomical career as a tour guide at the Griffith Observatory in Los Angeles.

His best known work was his catalogue of clusters of galaxies collected during the Palomar Sky Survey. He analyzed their formation and evolution. He demonstrated that second-order clustering existed, disproving the hierarchical model of Carl Charlier. He also discovered how cluster luminosity could be used as a distance scale. He also collated a famous list of 86 planetary nebula in 1966 which includes Abell 39.

The Abell catalogue is an almost complete list of approximately 4,000 clusters containing at least thirty members up to a redshift of z = 0.2. The original catalogue of clusters in the northern hemisphere was published in 1958. The extended catalogue, including clusters in the southern hemisphere, was published posthumously in 1989 in collaboration with Harold G. Corwin and Ronald P. Olowin.

Abell also co-discovered periodic comet 52P/Harrington-Abell. Together with Peter Goldreich, he correctly determined that planetary nebulae evolve from red giants.

Abell served for over twenty years as a faculty member at the Summer Science Program for high school students. The program memorializes him with its Abell Scholarship Fund. He was involved in the production of the educational TV series Understanding Space and Time and Project Universe.

Abell was passionate about debunking pseudoscientific claims such as those by Immanuel Velikovsky. He was a co-founder of the Committee on Scientific Investigation of Claims of the Paranormal (CSICOP) and contributed articles to their journal, The Skeptical Inquirer.

Abell served as president of the Cosmology Commission of the International Astronomical Union and as president of the Astronomical Society of the Pacific. He was elected a fellow of the Royal Astronomical Society in 1970. He was chairman of the UCLA Astronomy Department from 1968 to 1975 and chairman of the American Astronomical Society Education Committee. At the time of his death, he was to have become editor of the Astronomical Journal effective January 1, 1984.

Asteroid 3449 Abell is named in his honour, as is The George Abell Observatory at the Open University in Milton Keynes, England.